XENON1T S2 data constrain the solar scalar-electron coupling below 2e-15 at 90% CL, about three times weaker than the best stellar cooling bound.
OP data on CD for mean opacities and radiative accelerations
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
All monochromatic opacity data from the Opacity Project (OP), together with all codes required for the calculation of mean opacities and radiative accelerations for any required chemical mixture, temperature and mass-density, are being put on a 700 Mb CD which will be made generally available. The present paper gives a concise summary of the contents of the CD. More complete documentation will be provided on the CD itself.
citation-role summary
dataset 1
citation-polarity summary
fields
hep-ph 1years
2019 1verdicts
CONDITIONAL 1roles
dataset 1polarities
use dataset 1representative citing papers
citing papers explorer
-
Searching for a solar relaxion/scalar with XENON1T and LUX
XENON1T S2 data constrain the solar scalar-electron coupling below 2e-15 at 90% CL, about three times weaker than the best stellar cooling bound.